Petrogenesis of Lunar Rocks: Rb-Sr Constraints and Lack of H2O

Arden L Albee; Alexander J Gancarz

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NASA NTRS · 19780004987

Petrogenesis of Lunar Rocks: Rb-Sr Constraints and Lack of H2O

Arden L Albee·Alexander J Gancarz

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Abstract

Rb and Sr isotopic data and other chemical data indicate major lunar differentiation at about 4.6 AE (AE = 10 9 years) and very limited subsequent differentiation. The constraints of limited differentiation after 4.6 AE and the apparent lack of H20 on the Moon, when applied to the derivation and petrogenesis of lunar samples, suggest the following: (1) soil samples, breccias, metaclastic rocks, and feldspathic basalts represent mixtures of repeatedly modified clastic material, which was ultimately derived from materials formed during the ~ 4.6 AE differentiation; and (2) mare basalts crystallized from melts which formed by partial melting, and which developed without equilibration between the melt and crystalline residuum.

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Arden L Albee, Alexander J Gancarz. 1977-01-01. Petrogenesis of Lunar Rocks: Rb-Sr Constraints and Lack of H2O. https://ntrs.nasa.gov/citations/19780004987

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